This work is aimed at application of the Membrane Paradigm within the Parikh-Wilczek approach to rotating black holes. Developing pioneering researches on Electrodynamics and Gravitodynamics near black hole horizons [1]}, [2]} the Membrane Paradigm [3]}, [4]}, [5]}, [6]}, [7]} appeals to effective dynamics of a viscous fluid, simulated characteristics of a stretched membrane located at the horizon. Later on, the Duality between the hydrodynamic limit of a strongly coupled Gauge Theory and weakly coupled Gravity with matter was used for computing transport coefficients of the Gauge Theory on the Gravity side [8]}. Surprisingly, some of the results of the “old” Membrane Paradigm and of the “new” Gauge/Gravity Duality matched in the early development of the latter (see, e.g., [9]}, [10]}, [11]}). Notwithstanding that the Membrane Paradigm does not refer anyway to conformal symmetry, which plays the significant role as in the original AdS/CFT correspondence, as well as in its “light” version known as the Gauge/Gravity Duality.
